75 citations · 425 across the 18 of their papers we have counts for
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From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter
Hauke Koehn, Henrik Rose, Peter T. H. Pang +10
Through continuous progress in nuclear theory and experiment and an increasing number of neutron-star observations, a multitude of information about the equation of state (EOS) for…
What can we learn about the unstable equation-of-state branch from neutron-star mergers?
Maximiliano Ujevic, Rahul Somasundaram, Tim Dietrich +2
The Equation of State (EOS) of dense strongly-interacting matter can be probed by astrophysical observations of neutron stars (NS), such as X-ray detections of pulsars or the measu…
Impact of O4 future detection on the determination of the dense matter equations of state
J. -F. Coupechoux, R. Chierici, H. Hansen +3
In view of the next LIGO-Virgo-KAGRA Observing period O4 (to start in Spring 2023), we address the question of the ability of the interferometers network to discriminate among diff…
An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers
Peter T. H. Pang, Tim Dietrich, Michael W. Coughlin +18
The multi-messenger detection of the gravitational-wave signal GW170817, the corresponding kilonova AT2017gfo and the short gamma-ray burst GRB170817A, as well as the observed afte…
Impact of massive neutron star radii on the nature of phase transitions in dense matter
Rahul Somasundaram, Jérôme Margueron
The last few years have seen tremendous progress in the observation of the global properties of neutron stars (NSs), e.g. masses, radii and tidal deformabilities. Such properties p…